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Panoramic Spectroscopy of Sy Galaxies with elongated radio structures
Published online by Cambridge University Press: 01 August 2006
Abstract
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We have studied the ionized gas and stellar kinematics in several galaxies with active nuclei and elongated radio structures using 3D spectroscopy. The observations were performed at the SAO RAS 6-m telescope with the integral-field spectrograph MPFS (Afanasiev et al. 2001) and with a scanning Fabry-Perot interferometer (FPI) in the multimode device SCORPIO (Afanasiev & Moiseev 2005). Based on these data the intensity maps and velocity fields in the different emission lines of the ionizing gas were constructed. Using the lines-ratio diagrams we tried to search a source of the gas ionization: an active nucleus, hot young stars or shock waves.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 136
- Copyright
- Copyright © International Astronomical Union 2007
References
Afanasiev, V.L., Dodonov, S.N. & Moiseev, A.V. 2001, in: Osipkov, L.P. & Nikiforov, I.I. (eds.), Stellar dynamics: from classic to modern, p. 103.Google Scholar
Afanasiev, V.L. & Moiseev, A.V., 2005, Astron. Letters, 31, 193, astro-ph/0502095.CrossRefGoogle Scholar
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